Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Shah, Vishwangi"'
Autor:
Andrew, Shion, Leung, Calvin, Li, Alexander, Masui, Kiyoshi W., Andersen, Bridget C., Bandura, Kevin, Curtin, Alice P., Kaczmarek, Jane, Lanman, Adam E., Lazda, Mattias, Mena-Parra, Juan, Michilli, Daniele, Nimmo, Kenzie, Pearlman, Aaron B., Rahman, Mubdi, Shah, Vishwangi, Shin, Kaitlyn, Wang, Haochen
The Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project has a new VLBI Outrigger at the Green Bank Observatory (GBO), which forms a 3300km baseline with CHIME operating at 400-800MHz. Using 100ms long full-array baseba
Externí odkaz:
http://arxiv.org/abs/2409.11476
Autor:
Leung, Calvin, Andrew, Shion, Masui, Kiyoshi W., Brar, Charanjot, Cassanelli, Tomas, Chatterjee, Shami, Kaspi, Victoria, Khairy, Kholoud, Lanman, Adam E., Lazda, Mattias, Mena-Parra, Juan, Noble, Gavin, Pearlman, Aaron B., Rahman, Mubdi, Sanghavi, Pranav, Shah, Vishwangi
One major goal in fast radio burst science is to detect fast radio bursts (FRBs) over a wide field of view without sacrificing the angular resolution required to pinpoint them to their host galaxies. Wide-field detection and localization capabilities
Externí odkaz:
http://arxiv.org/abs/2403.05631
Autor:
Mckinven, Ryan, Bhardwaj, Mohit, Eftekhari, Tarraneh, Kilpatrick, Charles D., Kirichenko, Aida, Pal, Arpan, Cook, Amanda M., Gaensler, B. M., Giri, Utkarsh, Kaspi, Victoria M., Michilli, Daniele, Nimmo, Kenzie, Pearlman, Aaron B., Pleunis, Ziggy, Sand, Ketan R., Stairs, Ingrid, Andersen, Bridget C., Andrew, Shion, Bandura, Kevin, Brar, Charanjot, Cassanelli, Tomas, Chatterjee, Shami, Curtin, Alice P., Dong, Fengqiu Adam, Eadie, Gwendolyn, Fonseca, Emmanuel, Ibik, Adaeze L., Kaczmarek, Jane F., Kharel, Bikash, Lazda, Mattias, Leung, Calvin, Li, Dongzi, Main, Robert, Masui, Kiyoshi W., Mena-Parra, Juan, Ng, Cherry, Pandhi, Ayush, Patil, Swarali Shivraj, Prochaska, J. Xavier, Rafiei-Ravandi, Masoud, Scholz, Paul, Shah, Vishwangi, Shin, Kaitlyn, Smith, Kendrick
Fast radio bursts (FRBs) last for milliseconds and arrive at Earth from cosmological distances. While their origin(s) and emission mechanism(s) are presently unknown, their signals bear similarities with the much less luminous radio emission generate
Externí odkaz:
http://arxiv.org/abs/2402.09304
Autor:
Lanman, Adam E., Andrew, Shion, Lazda, Mattias, Shah, Vishwangi, Amiri, Mandana, Balasubramanian, Arvind, Bandura, Kevin, Boyle, P. J., Brar, Charanjot, Carlson, Mark, Cliche, Jean-François, Gusinskaia, Nina, Hendricksen, Ian T., Kaczmarek, J. F., Landecker, Tom, Leung, Calvin, Mckinven, Ryan, Mena-Parra, Juan, Milutinovic, Nikola, Nimmo, Kenzie, Pearlman, Aaron B., Renard, Andre, Rahman, Mubdi, Shaw, J. Richard, Siegel, Seth R., Smegal, Rick J., Cassanelli, Tomas, Chatterjee, Shami, Curtin, Alice P., Dobbs, Matt, Dong, Fengqiu Adam, Halpern, Mark, Hopkins, Hans, Kaspi, Victoria M., Khairy, Kholoud, Masui, Kiyoshi W., Meyers, Bradley W., Michilli, Daniele, Petroff, Emily, Pinsonneault-Marotte, Tristan, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Shin, Kaitlyn, Smith, Kendrick, Vanderlinde, Keith, Zegmott, Tarik J.
Localizing fast radio bursts (FRBs) to their host galaxies is an essential step to better understanding their origins and using them as cosmic probes. The CHIME/FRB Outrigger program aims to add VLBI-localization capabilities to CHIME, such that FRBs
Externí odkaz:
http://arxiv.org/abs/2402.07898
Autor:
Collaboration, The CHIME/FRB, Amiri, Mandana, Andersen, Bridget C., Andrew, Shion, Bandura, Kevin, Bhardwaj, Mohit, Boyle, P. J., Brar, Charanjot, Breitman, Daniela, Cassanelli, Tomas, Chawla, Pragya, Cook, Amanda M., Curtin, Alice P., Dobbs, Matt, Dong, Fengqiu Adam, Eadie, Gwendolyn, Fonseca, Emmanuel, Gaensler, B. M., Giri, Utkarsh, Herrera-Martin, Antonio, Hopkins, Hans, Ibik, Adaeze L., Joseph, Ronniy C., Kaczmarek, J. F., Kader, Zarif, Kaspi, Victoria M., Lanman, Adam E., Lazda, Mattias, Leung, Calvin, Liu, Siqi, Masui, Kiyoshi W., Mckinven, Ryan, Mena-Parra, Juan, Merryfield, Marcus, Michilli, Daniele, Ng, Cherry, Nimmo, Kenzie, Noble, Gavin, Pandhi, Ayush, Patel, Chitrang, Pearlman, Aaron B., Pen, Ue-Li, Petroff, Emily, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Rahman, Mubdi, Ransom, Scott M., Sand, Ketan R., Scholz, Paul, Shah, Vishwangi, Shin, Kaitlyn, Shpunarska, Yuliya, Siegel, Seth R., Smith, Kendrick, Stairs, Ingrid, Stenning, David C., Vanderlinde, Keith, Wang, Haochen, White, Henry, Wulf, Dallas
In 2021, a catalog of 536 fast radio bursts (FRBs) detected with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) radio telescope was released by the CHIME/FRB Collaboration. This large collection of bursts, observed with a single instrumen
Externí odkaz:
http://arxiv.org/abs/2311.00111
Autor:
Sand, Ketan R., Breitman, Daniela, Michilli, Daniele, Kaspi, Victoria M., Chawla, Pragya, Fonseca, Emmanuel, Mckinven, Ryan, Nimmo, Kenzie, Pleunis, Ziggy, Shin, Kaitlyn, Andersen, Bridget C., Bhardwaj, Mohit, Boyle, P. J., Brar, Charanjot, Cassanelli, Tomas, Cook, Amanda M., Curtin, Alice P., Dong, Fengqiu Adam, Eadie, Gwendolyn M., Gaensler, B. M., Kaczmarek, Jane, Lanman, Adam, Leung, Calvin, Masui, Kiyoshi W., Rahman, Mubdi, Pandhi, Ayush, Pearlman, Aaron B., Petroff, Emily, Rafiei-Ravandi, Masoud, Scholz, Paul, Shah, Vishwangi, Smith, Kendrick, Stairs, Ingrid, Stenning, David C.
FRB 20180916B is a repeating Fast Radio Burst (FRB) with a 16.3-day periodicity in its activity. In this study, we present morphological properties of 60 FRB 20180916B bursts detected by CHIME/FRB between 2018 August and 2021 December. We recorded ra
Externí odkaz:
http://arxiv.org/abs/2307.05839
Autor:
Sanghavi, Pranav, Leung, Calvin, Bandura, Kevin, Cassanelli, Tomas, Kaczmarek, Jane, Kaspi, Victoria M., Khairy, Kholoud, Lanman, Adam, Lazda, Mattias, Masui, Kiyoshi W., Mena-Parra, Juan, Michilli, Daniele, Pen, Ue-Li, Peterson, Jeffrey B., Rahman, Mubdi, Shah, Vishwangi
The sensitivity and field of view of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) has enabled its fast radio burst (FRB) backend to detect thousands of FRBs. However, the low angular resolution of CHIME prevents it from localizing most
Externí odkaz:
http://arxiv.org/abs/2304.10534
Autor:
Collaboration, The CHIME/FRB, Andersen, Bridget C., Bandura, Kevin, Bhardwaj, Mohit, Boyle, P. J., Brar, Charanjot, Cassanelli, Tomas, Chatterjee, S., Chawla, Pragya, Cook, Amanda M., Curtin, Alice P., Dobbs, Matt, Dong, Fengqiu Adam, Faber, Jakob T., Fandino, Mateus, Fonseca, Emmanuel, Gaensler, B. M., Giri, Utkarsh, Herrera-Martin, Antonio, Hill, Alex S., Ibik, Adaeze, Josephy, Alexander, Kaczmarek, Jane F., Kader, Zarif, Kaspi, Victoria, Landecker, T. L., Lanman, Adam E., Lazda, Mattias, Leung, Calvin, Lin, Hsiu-Hsien, Masui, Kiyoshi W., Mckinven, Ryan, Mena-Parra, Juan, Meyers, Bradley W., Michilli, D., Ng, Cherry, Pandhi, Ayush, Pearlman, Aaron B., Pen, Ue-Li, Petroff, Emily, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Rahman, Mubdi, Ransom, Scott M., Renard, Andre, Sand, Ketan R., Sanghavi, Pranav, Scholz, Paul, Shah, Vishwangi, Shin, Kaitlyn, Siegel, Seth, Smith, Kendrick, Stairs, Ingrid, Su, Jianing, Tendulkar, Shriharsh P., Vanderlinde, Keith, Wang, Haochen, Wulf, Dallas, Zwaniga, Andrew
We present the discovery of 25 new repeating fast radio burst (FRB) sources found among CHIME/FRB events detected between 2019 September 30 and 2021 May 1. The sources were found using a new clustering algorithm that looks for multiple events co-loca
Externí odkaz:
http://arxiv.org/abs/2301.08762
Multi-mode Cepheids pulsate simultaneously in more than one mode of oscillation. They provide an independent means to test stellar models and pulsation theories. They can also be used to derive metallicities. In recent years, the number of known mult
Externí odkaz:
http://arxiv.org/abs/2208.03080